天鹅座BC
| 观测资料 历元 J2000 | |
|---|---|
| 星座 | 天鹅座 |
| 星官 | |
| 赤经 | 20h 21m 38.55s[1] |
| 赤纬 | 37° 31′ 58.9″[1] |
| 视星等（V） | 9.0 - 10.8[2] |
| 特性 | |
| 光谱分类 | M3.5 Ia[3] (M2 - M5[4]) |
| B−V 色指数 | +3.13 - +3.21[4] |
| 变星类型 | SRc[3] |
| 天体测定 | |
| 径向速度 (Rv) | −20.97[1] km/s |
| 自行 (μ) | 赤经：−3.710[1] mas/yr 赤纬：−6.307[1] mas/yr |
| 视差 (π) | 0.5760 ± 0.0500[1] mas |
| 距离 | 1,710+40 −40[5] pc |
| 绝对星等 (MV) | −7.71[6] |
| 详细资料 [4] | |
| 质量 | 19 M☉ |
| 半径 | 1,031[7] R☉ |
| 亮度 | 204,000[5] L☉ |
| 温度 | 3,605[8] K |
| Minimum (1900) | |
| 半径 | 1,553 R☉ |
| 亮度 | 145,000 L☉ |
| 温度 | 2,858 K |
| Maximum (2000) | |
| 半径 | 856 R☉ |
| 亮度 | 112,000 L☉ |
| 温度 | 3,614 K |
| 其他命名 | |
| 参考资料库 | |
| SIMBAD | 资料 |
天鹅座BC（BC Cyg, HIP 100404, BD + 37 3903）是在天鹅座的一颗光谱类型M3.5Ia 红超巨星和脉动变星。
它被认为是天鹅座OB1星协的成员，其中有疏散星团伯克利87[9]，位于距离太阳系1,673秒差距（5,000光年）之处[10]。它位于另一个红超巨星天鹅座BI以北不到一度的地方[来源请求]。根据其盖亚目录的视差，它的距离大约在1,700 pc.[1]。
计算得到天鹅座BC的有效温度在2,858至3,614K，并且光度在112,000到145,000 L☉之间变化。最亮和最冷时的大小被计算为1,553 R☉，而最热和最暗时的大小为856 R☉。它是已知最大的恒星之一。如果它取代太阳的位置，假设最大半径为1553 R☉，其光球将吞噬木星的轨道。其质量约为19 M☉，据估计，恒星质量损失，如尘埃，原子和分子气体为每年3.2×10−9 M☉[11]。
天鹅座BC的视星等在+9.0 and +10.8之间变化，周期为720 ± 40日[2]。大约在1900年至2000年之间，它的平均亮度似乎增加了0.5星等[4]。
相关条目
[编辑]参考资料
[编辑]- ^ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 Vallenari, A.; et al. Gaia Data Release 3. Summary of the content and survey properties. Astronomy & Astrophysics. 2022. arXiv:2208.00211
. doi:10.1051/0004-6361/202243940 . 已忽略未知参数|collaboration=(帮助) Gaia DR3 record for this source at VizieR. - ^ 2.0 2.1 Kiss, L. L.; Szabó, Gy. M.; Bedding, T. R. Variability in red supergiant stars: Pulsations, long secondary periods and convection noise. Monthly Notices of the Royal Astronomical Society. 2006, 372 (4): 1721–1734. Bibcode:2006MNRAS.372.1721K. S2CID 5203133. arXiv:astro-ph/0608438 . doi:10.1111/j.1365-2966.2006.10973.x.
- ^ 3.0 3.1 Samus, N. N.; Durlevich, O. V.; et al. VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013). VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S. 2009, 1. Bibcode:2009yCat....102025S.
- ^ 4.0 4.1 4.2 4.3 Turner, David G.; Rohanizadegan, Mina; Berdnikov, Leonid N.; Pastukhova, Elena N. The Long-Term Behavior of the Semiregular M Supergiant Variable BC Cygni. The Publications of the Astronomical Society of the Pacific. 2006, 118 (849): 1533. Bibcode:2006PASP..118.1533T. doi:10.1086/508905 .
- ^ 5.0 5.1 Davies, Ben; Beasor, Emma R. The 'red supergiant problem': the upper luminosity boundary of Type II supernova progenitors. MNRAS. March 2020, 493 (1): 468–476. Bibcode:2020MNRAS.493..468D. S2CID 210714093. arXiv:2001.06020 . doi:10.1093/mnras/staa174 （英语）.
- ^ Levesque, Emily M.; Massey, Philip; Olsen, K. A. G.; Plez, Bertrand; Josselin, Eric; Maeder, Andre; Meynet, Georges. The Effective Temperature Scale of Galactic Red Supergiants: Cool, but Not As Cool As We Thought. The Astrophysical Journal. 2005, 628 (2): 973–985. Bibcode:2005ApJ...628..973L. S2CID 15109583. arXiv:astro-ph/0504337 . doi:10.1086/430901.
- ^ Comerón, F.; Djupvik, A. A.; Schneider, N.; Pasquali, A. The historical record of massive star formation in Cygnus. Astronomy & Astrophysics. October 2020, 2009: A62. Bibcode:2020A&A...644A..62C. S2CID 221970180. arXiv:2009.12779 . doi:10.1051/0004-6361/202039188.
- ^ Messineo, M.; Brown, A. G. A. A Catalog of Known Galactic K-M Stars of Class I Candidate Red Supergiants in Gaia DR2. The Astronomical Journal. 2019, 158 (1): 20. Bibcode:2019AJ....158...20M. S2CID 148571616. arXiv:1905.03744 . doi:10.3847/1538-3881/ab1cbd.
- ^ Sokal, Kimberly R.; Skinner, Stephen L.; Zhekov, Svetozar A.; Güdel, Manuel; Schmutz, Werner. Chandra Detects the Rare Oxygen-type Wolf-Rayet Star WR 142 and OB Stars in Berkeley 87. The Astrophysical Journal. 2010, 715 (2): 1327. Bibcode:2010ApJ...715.1327S. S2CID 119232391. arXiv:1004.0462 . doi:10.1088/0004-637X/715/2/1327.
- ^ de la Fuente, Diego; Román-Zúñiga, Carlos G.; Jiménez-Bailón, Elena; Alves, João; Garcia, Miriam; Venus, Sean. Clustered star formation toward Berkeley 87/ON2. I. Multiwavelength census and the population overlap problem. Astronomy and Astrophysics. 2021, 650: A156. Bibcode:2021A&A...650A.156D. S2CID 232170603. arXiv:2103.06062 . doi:10.1051/0004-6361/202040065.
- ^ Josselin, E.; Plez, B. Atmospheric dynamics and the mass loss process in red supergiant stars. Astronomy and Astrophysics. 2007, 469 (2): 671. Bibcode:2007A&A...469..671J. S2CID 17789027. arXiv:0705.0266 . doi:10.1051/0004-6361:20066353.
- ^ Download Data. aavso.org. AAVSO. [1 October 2021]. （原始内容存档于2023-03-15）.
